Mathematics
Scientific paper
Feb 1984
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984ge%26ae..24...89l&link_type=abstract
Geomagnetizm i Aeronomiia (ISSN 0016-7940), vol. 24, Jan.-Feb. 1984, p. 89-93. In Russian.
Mathematics
3
Auroras, Earth Magnetosphere, Polar Substorms, Space Plasmas, Convexity, Electric Field Strength, Field Aligned Currents, Hall Effect, Mathematical Models, Plasma Heating, Plasma-Electromagnetic Interaction
Scientific paper
The poleward motion of the auroral convexity is explained by the heating of the magnetospheric plasma inside a region of field-aligned currents and longitudinal potential-difference. The heated magnetospheric plasma moves away from the earth. If the Hall conductivity of the ionosphere below the heated-plasma region increases, the polarization electric-field inside this region acquires a poleward component, and the velocity of the heated region acquires a westward component. Expected poleward velocities of the heated plasma agree with observed velocities of the auroral convexity and amount to several km/s at the ionospheric level.
Liatskii V. B.
Maltsev Iu. P.
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